HIP 74507
HIP 74507 is a K-type (Orange) star.
At a distance of roughly 1,382 light-years, HIP 74507 is a distant star lying deep within the Milky Way galaxy.
HIP 74507 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 74507 has an apparent magnitude of +8.73, placing it beyond naked-eye visibility. A good pair of binoculars or a small telescope is required to observe this star. Observers will note its orange hue, which corresponds to a B-V color index of +1.090.
Physical Properties
| Spectral Class | K Class K — K-type (Orange) |
| Color Index (B−V) | 1.090 |
Observation
| Apparent Magnitude | +8.73 |
| Absolute Magnitude | 0.60 |
| Distance | 1,382 ly |
Position
| Right Ascension | 15h 13.53m |
| Declination | 15° 55.34′ |
Frequently Asked Questions
What type of star is HIP 74507?
HIP 74507 is a Class K — K-type (Orange) star.
How far is HIP 74507 from Earth?
HIP 74507 is approximately 1,382.0 light-years from Earth.
Can you see HIP 74507 with the naked eye?
With an apparent magnitude of 8.73, HIP 74507 is not visible to the naked eye.